Emission and flux of DMS from the Australian Antarctic and Subantarctic Oceans during the 1988/89 summer
Identifieur interne : 000841 ( Istex/Corpus ); précédent : 000840; suivant : 000842Emission and flux of DMS from the Australian Antarctic and Subantarctic Oceans during the 1988/89 summer
Auteurs : A. R. Mctaggart ; H. R. Burton ; B. C. NguyenSource :
- Journal of Atmospheric Chemistry [ 0167-7764 ] ; 1995-01-01.
English descriptors
- KwdEn :
- Andreae, Antarctic, Antarctic continent, Antarctic convergence, Antarctic divergence, Antarctic ocean, Austral summer, Australasian, Australasian antarctic, Australasian antarctic ocean, Australasian sector, Divergence, Geophys, January, Mctaggart, Nguyen, November, Offshelf waters, Piston velocity, Schmidt number, Seawater, Southern ocean, Subantarctic, Subantarctic ocean, Subantarctic oceans, Water masses, Wind speed, Wind speeds.
- Teeft :
- Andreae, Antarctic, Antarctic continent, Antarctic convergence, Antarctic divergence, Antarctic ocean, Austral summer, Australasian, Australasian antarctic, Australasian antarctic ocean, Australasian sector, Divergence, Geophys, January, Mctaggart, Nguyen, November, Offshelf waters, Piston velocity, Schmidt number, Seawater, Southern ocean, Subantarctic, Subantarctic ocean, Subantarctic oceans, Water masses, Wind speed, Wind speeds.
Abstract
Abstract: DMS emissions and fluxes from the Australasian sector of the Antarctic and Subantarctic Oceans, bound by 46–68° S and 65.5–142.6° E, were determined from a limited number of samples (n=32) collected during three summer resupply voyages to Australian Antarctic continental research bases between November 1988 and January 1989 (a 92 day period). The maximum DMS emission from this sector of the Antarctic Ocean was in an area near the Antarctic Divergence (60–63° S) and the minimum DMS emission was from the Antarctic coastal and offshelf waters. The greatest emission of DMS from this sector of the Southern Ocean was from the Subantarctic waters. DMS flux from the Australasian Antarctic Ocean was 64.3×106 (±115) mol d−1 or 5.9 (±10.6)×109 mol based on an emission of 10.9 (±19.5) µmol m−2 d−1 (n=26). The flux of DMS from the Australasian sector of the Subantarctic Ocean was probably twice the flux of DMS from the adjacent Antarctic Ocean.
Url:
DOI: 10.1007/BF01099918
Links to Exploration step
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<front><div type="abstract" xml:lang="en">Abstract: DMS emissions and fluxes from the Australasian sector of the Antarctic and Subantarctic Oceans, bound by 46–68° S and 65.5–142.6° E, were determined from a limited number of samples (n=32) collected during three summer resupply voyages to Australian Antarctic continental research bases between November 1988 and January 1989 (a 92 day period). The maximum DMS emission from this sector of the Antarctic Ocean was in an area near the Antarctic Divergence (60–63° S) and the minimum DMS emission was from the Antarctic coastal and offshelf waters. The greatest emission of DMS from this sector of the Southern Ocean was from the Subantarctic waters. DMS flux from the Australasian Antarctic Ocean was 64.3×106 (±115) mol d−1 or 5.9 (±10.6)×109 mol based on an emission of 10.9 (±19.5) µmol m−2 d−1 (n=26). The flux of DMS from the Australasian sector of the Subantarctic Ocean was probably twice the flux of DMS from the adjacent Antarctic Ocean.</div>
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<abstract>Abstract: DMS emissions and fluxes from the Australasian sector of the Antarctic and Subantarctic Oceans, bound by 46–68° S and 65.5–142.6° E, were determined from a limited number of samples (n=32) collected during three summer resupply voyages to Australian Antarctic continental research bases between November 1988 and January 1989 (a 92 day period). The maximum DMS emission from this sector of the Antarctic Ocean was in an area near the Antarctic Divergence (60–63° S) and the minimum DMS emission was from the Antarctic coastal and offshelf waters. The greatest emission of DMS from this sector of the Southern Ocean was from the Subantarctic waters. DMS flux from the Australasian Antarctic Ocean was 64.3×106 (±115) mol d−1 or 5.9 (±10.6)×109 mol based on an emission of 10.9 (±19.5) µmol m−2 d−1 (n=26). The flux of DMS from the Australasian sector of the Subantarctic Ocean was probably twice the flux of DMS from the adjacent Antarctic Ocean.</abstract>
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<ArticleTitle Language="En">Emission and flux of DMS from the Australian Antarctic and Subantarctic Oceans during the 1988/89 summer</ArticleTitle>
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<Author AffiliationIDS="Aff3"><AuthorName DisplayOrder="Western"><GivenName>B.</GivenName>
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<FamilyName>Nguyen</FamilyName>
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<Affiliation ID="Aff1"><OrgDivision>Australian Antarctic Division</OrgDivision>
<OrgName>Channel Highway</OrgName>
<OrgAddress><Postcode>7150</Postcode>
<City>Kingston</City>
<State>Tasmania</State>
<Country>Australia</Country>
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<Affiliation ID="Aff3"><OrgDivision>Centre des Faibles Radioactivites</OrgDivision>
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<City>Gif sur Yvette Cedex</City>
<Country>France</Country>
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<Affiliation ID="Aff2"><OrgDivision>Biogeochemical Laboratories, Geology 307</OrgDivision>
<OrgName>Indiana University</OrgName>
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<City>Bloomington</City>
<State>IN</State>
<Country>USA</Country>
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<Para>DMS emissions and fluxes from the Australasian sector of the Antarctic and Subantarctic Oceans, bound by 46–68° S and 65.5–142.6° E, were determined from a limited number of samples (<Emphasis Type="Italic">n</Emphasis>
=32) collected during three summer resupply voyages to Australian Antarctic continental research bases between November 1988 and January 1989 (a 92 day period). The maximum DMS emission from this sector of the Antarctic Ocean was in an area near the Antarctic Divergence (60–63° S) and the minimum DMS emission was from the Antarctic coastal and offshelf waters. The greatest emission of DMS from this sector of the Southern Ocean was from the Subantarctic waters. DMS flux from the Australasian Antarctic Ocean was 64.3×10<Superscript>6</Superscript>
(±115) mol d<Superscript>−1</Superscript>
or 5.9 (±10.6)×10<Superscript>9</Superscript>
mol based on an emission of 10.9 (±19.5) µmol m<Superscript>−2</Superscript>
d<Superscript>−1</Superscript>
(<Emphasis Type="Italic">n</Emphasis>
=26). The flux of DMS from the Australasian sector of the Subantarctic Ocean was probably twice the flux of DMS from the adjacent Antarctic Ocean.</Para>
</Abstract>
<KeywordGroup Language="En"><Heading>Key words</Heading>
<Keyword>DMS</Keyword>
<Keyword>emission and flux</Keyword>
<Keyword>Australasian Antarctic and Subantarctic Oceans</Keyword>
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<abstract lang="en">Abstract: DMS emissions and fluxes from the Australasian sector of the Antarctic and Subantarctic Oceans, bound by 46–68° S and 65.5–142.6° E, were determined from a limited number of samples (n=32) collected during three summer resupply voyages to Australian Antarctic continental research bases between November 1988 and January 1989 (a 92 day period). The maximum DMS emission from this sector of the Antarctic Ocean was in an area near the Antarctic Divergence (60–63° S) and the minimum DMS emission was from the Antarctic coastal and offshelf waters. The greatest emission of DMS from this sector of the Southern Ocean was from the Subantarctic waters. DMS flux from the Australasian Antarctic Ocean was 64.3×106 (±115) mol d−1 or 5.9 (±10.6)×109 mol based on an emission of 10.9 (±19.5) µmol m−2 d−1 (n=26). The flux of DMS from the Australasian sector of the Subantarctic Ocean was probably twice the flux of DMS from the adjacent Antarctic Ocean.</abstract>
<relatedItem type="host"><titleInfo><title>Journal of Atmospheric Chemistry</title>
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